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Related papers: Distances of Dwarf Carbon Stars

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Our understanding of large amplitude pulsating stars and their status in stellar evolution is briefly reviewed. The paper then describes the near-infrared light curves of various asymptotic giant branch stars, concentrating on possible…

Astrophysics · Physics 2007-05-23 Patricia A. Whitelock

Brown dwarfs and giant planets orbiting close to a host star are subjected to significant irradiation that can modify the properties of their atmospheres. In order to test the atmospheric models that are used to describe these systems, it…

Numerous white dwarf stars are known to be orbited by disks of gas and dust. To date, broad, about 300 km s-1 wide, gaseous circumstellar absorption features have only been reported for the already iconic WD 1145+017, where one is…

Wide binaries are tracers of the gravity field of the Galaxy, but their study requires some caution. A large list of common proper motion stars selected from the AGK3 were monitored with the CORAVEL spectrovelocimeter, in order to prepare a…

Solar and Stellar Astrophysics · Physics 2011-12-12 Jean-Louis Halbwachs , Michel Mayor , Stéphane Udry

We report new results of our search for rare, cool carbon stars located at large distances from the galactic plane. Eighteen new C stars were discovered. Six are remarkable by showing the two peculiarities of a strong infrared excess at 12…

Astrophysics · Physics 2010-04-21 Nicolas Mauron

We present a detailed study of radio-detected dwarf galaxies (with stellar masses less than 3 billion solar masses) to characterize extreme star formation and search for (variable) radio AGNs. Our sample comes from Reines et al. (2020)…

Astrophysics of Galaxies · Physics 2026-05-01 John-Michael Eberhard , Amy E. Reines

With its exquisite astrometric precision, the latest Gaia data release includes $\sim$$10^5$ astrometric binaries, each of which have measured orbital periods, eccentricities, and the Thiele-Innes orbital parameters. Using these and an…

Solar and Stellar Astrophysics · Physics 2022-07-05 Jeff J. Andrews , Kirsty Taggart , Ryan Foley

The dwarf carbon (dC) star SDSS J112801.67+004034.6 has an unusually high radial velocity, 531$\pm 4$ km s$^{-1}$. We present proper motion and new spectroscopic observations which imply a large Galactic rest frame velocity, 425$\pm 9$ km…

Solar and Stellar Astrophysics · Physics 2016-12-28 Kathryn A. Plant , Bruce Margon , Puragra Guhathakurta , Emily C. Cunningham , Elisa Toloba , Jeffrey A. Munn

We have conducted a novel search of most of the southern sky for nearby red dwarfs having low proper motions, with specific emphasis on those with proper motion < 0.18 arcsec yr-1, the lower cutoff of Luyten's classic proper motion catalog.…

Using Gaia DR2 data, we present an up-to-date sample of white dwarfs within 20 pc of the Sun. In total we identified 139 systems in Gaia DR2, nine of which are new detections, with the closest of these located at a distance of 13.05 pc. We…

Solar and Stellar Astrophysics · Physics 2018-08-15 M. A. Hollands , P. E. Tremblay , B. T. Gaensicke , N. P. Gentile-Fusillo , S. Toonen

Multiple radial velocity observations have been obtained for a large sample of local field subdwarf B (sdB) stars over a period of two years. SdB stars appear to fall into three distinct groups based on their kinematic and spectroscopic…

Astrophysics · Physics 2007-05-23 Rex A. Saffer , Elizabeth M. Green , Timothy P. Bowers

Optical linear polarimetry of 8 ultra cool field dwarfs, with spectral types ranging from M9 to L8, is presented. The linear polarisation, P, of each dwarf we measured is P < 0.2%. Three dwarfs have polarisations compatible with zero, two…

Astrophysics · Physics 2009-11-07 Francois Menard , Xavier Delfosse , Jean-Louis Monin

We present the first results of a new survey for finding cool N-type carbon (C) stars in the halo of the Galaxy. Candidates were first selected in the 2MASS Second Incremental Release database with JHKs colours typical of red AGB C stars…

Astrophysics · Physics 2009-11-10 N. Mauron , M. Azzopardi , K. Gigoyan , T. R. Kendall

Carbon stars are excellent kinematic tracers of galaxies and play important roles in understanding the evolution of the Galaxy. Therefore, it is worthwhile to search for them in a large amount of spectra. In this work, we build a new carbon…

Astrophysics of Galaxies · Physics 2023-12-12 Linlin Li , Kecheng Zhang , Wenyuan Cui , Jianrong Shi , Wei Ji , Zhenyan Huo , Yawei Gao , Shuai Zhang , Mingxu Sun

28 hitherto neglected candidates for the Catalogue of Nearby Stars (CNS) were investigated to verify their classification and to improve their distance estimates. All targets had at least a preliminary status of being nearby dwarf stars…

Astrophysics · Physics 2009-11-13 H. Jahreiss , H. Meusinger , R. -D. Scholz , B. Stecklum

We present an analysis of the chemical abundances and kinematics of six low-mass dwarf stars, previously claimed to be candidate hypervelocity stars (HVSs). We obtained moderate-resolution ($R\sim$ 6000) spectra of these stars to estimate…

Astrophysics of Galaxies · Physics 2019-07-17 Bum-Suk Yeom , Young Sun Lee , Jae-Rim Koo , Timothy C. Beers , Young Kwang Kim

In this study, we explore the characteristics of carbon stars within our Galaxy through a comprehensive analysis of observational data spanning visual and infrared (IR) bands. Leveraging datasets from IRAS, ISO, Akari, MSX, 2MASS, WISE,…

Solar and Stellar Astrophysics · Physics 2024-03-28 Kyung-Won Suh

Data on the multiplicity of F- and G-type dwarf stars within 67pc of the Sun are presented. This distance-limited sample based on the Hipparcos catalog contains 4847 primary stars (targets) with 0.5<V-I_C<0.8 and is >90% complete. There are…

Solar and Stellar Astrophysics · Physics 2015-06-18 Andrei Tokovinin

Five nearby dwarf irregular galaxies, amongst the recently surveyed dwarf members of the Sculptor and Centaurus A groups (at 2.5 Mpc and 3.5 Mpc), have been imaged in neutral hydrogen (HI) with the Australia Telescope and the Very Large…

Astrophysics · Physics 2007-05-23 Stephanie Cote , Ken Freeman , Claude Carignan

Although carbon is, together with oxygen and nitrogen, one of the most important elements in the study of galactic chemical evolution its production sites are still poorly known and have been much debated (see e.g. Gustafsson et al. 1999;…

Astrophysics · Physics 2009-11-11 T. Bensby , S. Feltzing
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